Image Processing Reference
In-Depth Information
Image-Stabilization Systems
Figure 7.2 Picture of MACAO wavefront sensor package. Light from the telescope is
coming from the top.
Hubin, N.N., “Adaptive optics status and roadmap at ESO,” Proceedings of
SPIE , 5490 , 195-206 (2004).
Bonaccini, D., F.J. Rigaut, G. Dudziak, G. Monnet, “Curvature adaptive optics
at ESO,” Proceedings of SPIE , 3353 , 553-560 (1998).
Gemini Observatory
The Gemini Observatory is composed of two 8-m aperture telescopes, one located
at Cerro Pachon in Chile (Gemini South) and the other on Mauna Kea on Hawaii
(Gemini North). Gemini North has a natural guide star system called Altair that has
a 177-actuator, deformable mirror, and a separate tip-tilt mirror.
McGregor, P., J. Hart, D. Stevanovic, G. Bloxham, D. Jones, J. Van Harmelen,
J. Griesbach, M. Dawson, P. Young, M.A. Jarnyk, “Gemini South adaptive op-
tics imager (GSAOI),” Proceedings of SPIE , 5492 , 1033-1044 (2004).
Meeks, R.L., J. Lopez, M. Nickerson, G. Pentland, C. Smith, A. Rakich, “Pre-
liminary optomechanical design and analysis of the Gemini multiconjugate
adaptive optics bench,” Proceedings of SPIE , 5490 , 289-298 (2004).
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